LEADER 03708nam 22006375 450 001 9910300409603321 005 20200629115930.0 010 $a3-319-09540-4 024 7 $a10.1007/978-3-319-09540-0 035 $a(CKB)3710000000227360 035 $a(EBL)1968643 035 $a(OCoLC)908090185 035 $a(SSID)ssj0001338807 035 $a(PQKBManifestationID)11704407 035 $a(PQKBTitleCode)TC0001338807 035 $a(PQKBWorkID)11345035 035 $a(PQKB)10140195 035 $a(DE-He213)978-3-319-09540-0 035 $a(MiAaPQ)EBC1968643 035 $a(PPN)180628178 035 $a(EXLCZ)993710000000227360 100 $a20140830d2015 u| 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aNumerical Simulation of Viscous Shocked Accretion Flows Around Black Holes /$fby Kinsuk Giri 205 $a1st ed. 2015. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2015. 215 $a1 online resource (148 p.) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 300 $aDescription based upon print version of record. 311 $a3-319-09539-0 320 $aIncludes bibliographical references. 327 $aIntroduction -- Overview of Numerical Simulations on Accretion Processes and Our Objectives -- Governing Equations and Computational Methods -- Simulation Procedure and the Test of the Code -- Simulation for Inviscid Sub-Keplerian Flows and Shocks -- Simulation of Viscous Accretion Flows -- Effects of Power-law Cooling in Viscous Flows -- Conclusions and Future Plans. 330 $aThe work developed in this thesis addresses very important and relevant issues of accretion processes around black holes. Beginning by studying the time variation of the evolution of inviscid accretion discs around black holes, and their properties, the author investigates the change of the pattern of the flows when the strength of the shear viscosity is varied and cooling is introduced. He succeeds to verify theoretical predictions of the so called Two Component Advective Flow (TCAF) solution of the accretion problem onto black holes through numerical simulations under different input parameters. TCAF solutions are found to be stable. And thus explanations of spectral and timing properties (including Quasi-Period Oscillations, QPOs) of galactic and extra-galactic black holes based on shocked TCAF models appear to have a firm foundation. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aAstrophysics 606 $aMathematical physics 606 $aComputer science$xMathematics 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aTheoretical, Mathematical and Computational Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P19005 606 $aComputational Mathematics and Numerical Analysis$3https://scigraph.springernature.com/ontologies/product-market-codes/M1400X 615 0$aAstrophysics. 615 0$aMathematical physics. 615 0$aComputer science$xMathematics. 615 14$aAstrophysics and Astroparticles. 615 24$aTheoretical, Mathematical and Computational Physics. 615 24$aComputational Mathematics and Numerical Analysis. 676 $a523.8875015118 700 $aGiri$b Kinsuk$4aut$4http://id.loc.gov/vocabulary/relators/aut$0792328 906 $aBOOK 912 $a9910300409603321 996 $aNumerical Simulation of Viscous Shocked Accretion Flows Around Black Holes$91771650 997 $aUNINA